activity
19932025
most citedThe Demography of Massive Dark Objects in Galaxy Centres

4k citations · 40.2k across the 165 of their papers we have counts for

collaborators
Showing 2016Show all

8 papers · 1 filter

astro-ph.IM2016★ 236 cited

The DESI Experiment Part II: Instrument Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…

astro-ph.IM2016★ 1.3k cited

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…

astro-ph.EP2016★ 21 cited

The First High-Phase Observations of a KBO: New Horizons Imaging of (15810) 1994 JR1 from the Kuiper Belt

Simon B. Porter, John R. Spencer, Susan Benecchi +12

NASA's New Horizons spacecraft observed (15810) 1994 JR, a 3:2 resonant Kupier Belt Object (KBO), using the LOng Range Reconnaissance Imager (LORRI) on November 2, 2015 from a…

astro-ph.EP2016★ 271 cited

The Geology of Pluto and Charon Through the Eyes of New Horizons

Jeffrey M. Moore, William B. McKinnon, John R. Spencer +38

NASA's New Horizons spacecraft has revealed the complex geology of Pluto and Charon. Pluto's encounter hemisphere shows ongoing surface geological activity centered on a vast basin…

astro-ph.EP2016★ 94 cited

The Small Satellites of Pluto as Observed by New Horizons

H. A. Weaver, M. W. Buie, B. J. Buratti +48

The New Horizons mission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra. All four are small, with equivalent spherical diameters of 40…

astro-ph.GA2016★ 24 cited

High-Resolution Mapping of Dust via Extinction in the M31 Bulge

Hui Dong, Zhiyuan Li, Q. D. Wang +5

We map the dust distribution in the central 180" (~680 pc) region of the M31 bulge, based on HST/WFC3 and ACS observations in ten bands from near-ultraviolet (2700 A) to near-infra…